The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 39 Issue 2
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- Pages.99.2-99.2
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- 2014
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- 1226-2692(pISSN)
A model of a solar eruption affected by a solar wind
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Lee, Hwanhee
(School of Space Research, Kyung Hee University)
;
- Magara, Tetsuya (School of Space Research, Kyung Hee University) ;
- Kang, Jihye (School of Space Research, Kyung Hee University) ;
- Satoshi, Inoue (School of Space Research, Kyung Hee University) ;
- An, Jun-Mo (School of Space Research, Kyung Hee University)
- Published : 2014.10.13
Abstract
We investigate how a solar eruption occurs in an environment where a solar wind exists during a pre-eruptive phase. To understand it, we have performed three-dimensional simulations based on a zero-beta magnetohydrodynamic (MHD) equations in various ways to drive an eruption with a solar wind. A pre-eruptive state is derived by applying a nonlinear force-free reconstruction method to a flux emergence full MHD simulation. We discuss what is the most appropriate way to drive a solar wind-related eruption.
Keywords